HD 121056

HD 121056, or HIP 67851, is an aging giant star with a pair of orbiting exoplanets located in the southern constellation of Centaurus. This star is dimly visible to the naked eye with an apparent visual magnitude of 6.17. It is located at a distance of 209 light years from the Sun, based on parallax measurements, and is drifting further away with a radial velocity of 5.6 km/s.

HD 121056
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 13h 53m 52.06131s
Declination −35° 18 51.6918
Apparent magnitude (V) 6.17
Characteristics
Evolutionary stage giant star
Spectral type K0 III
B−V color index 1.01
Astrometry
Radial velocity (Rv)5.60±0.13 km/s
Proper motion (μ) RA: −295.304±0.040 mas/yr
Dec.: −68.458±0.058 mas/yr
Parallax (π)15.6261 ± 0.0418 mas
Distance208.7 ± 0.6 ly
(64.0 ± 0.2 pc)
Absolute magnitude (MV)+2.08
Details
Mass1.60±0.18 M
Radius5.72 R
Luminosity15.8 L
Surface gravity (log g)3.261±0.105 cgs
Temperature4,867±49 K
Metallicity[Mg/H] 0.286±0.05 dex
Metallicity [Fe/H]0.020±0.031 dex
Rotational velocity (v sin i)2.38±0.51 km/s
Age5.46 Gyr
Other designations
CD−34 9223, Gaia DR2 6169943210465504384, GJ 532.1, HD 121056, HIP 67851, HR 5224, TYC 7287-1874-1, 2MASS J13535209-3518517
Database references
SIMBADdata

The spectrum of HD 121056 presents as an evolved K-type giant star with a stellar classification of K0 III. It is presently ascending the red-giant branch, having exhausted the supply of hydrogen at its core. The star is about 5.5 billion years old and is spinning with a projected rotational velocity of 2.4 km/s. HD 121056’s concentration of heavy elements is similar to the Sun, with a metallicity Fe/H index of 0.020±0.031, although the star is enriched in lighter rock-forming elements like magnesium and aluminum. It has 1.6 times the mass of the Sun and has expanded to 5.72 times the Sun's radius. The star is radiating 15.8 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,867 K.

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